Difference between revisions of "03/30/2011 01:00:00 UTC"
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**Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source | **Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source | ||
**There is no apparent halo-like feature as seen from LASCO | **There is no apparent halo-like feature as seen from LASCO | ||
| + | <br /> | ||
| + | * Is the CME over-expanding (Gosling et al. )? pressure profile needed | ||
| + | |||
==In-Situ Data== | ==In-Situ Data== | ||
A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| − | [[File: | + | [[File:plot_sw_mag_plasma_2011032900.png|350px]] |
| − | [[File: | + | [[File:plot_sw_mag_2011032900.png|400px]] |
| − | [[File: | + | [[File:plot_sw_vel_2011032900.png|350px]] <br /> |
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
Latest revision as of 12:36, 2 July 2013
Comment Section
- A slow ICME with extremely long duration as seen at 1 AU
- Seems an excellent example of the so-called "global" CME, or longitudinal extended CME (Jie)
- COR2 A: symmetric above both east and west limbs along the equator, indicating a global feature
- COR2 B: same as COR2, symmetric above both limbs
- Combining COR2 A and B, it seems a global CME, surrounding the entire solar equator
- Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source
- There is no apparent halo-like feature as seen from LASCO
- Is the CME over-expanding (Gosling et al. )? pressure profile needed
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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Error creating thumbnail: File missing
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
GOES X-RAY FLUX
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The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.
